RMS Images are meant to represent the root-mean-square deviation from the mean (rmsd) appropriate to measure the noise level in a Gaussian distribution.

maximum 5.4527e-04 Jy/beam
minimum 1.0735e-04 Jy/beam
mean 1.6961e-04 Jy/beam
median 1.2903e-04 Jy/beam
sigma 8.2009e-05 Jy/beam
MAD rms 1.3683e-05 Jy/beam

RMS images

TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms

Pilot.ql.SGC3B_1.J235401_124236.10.2048.v1.I.iter1.image.pbcor.tt0.rms.sky.png

No pipeline QA for this task.
vis
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3B_1.J235401+124236_P30566v1_2019_01_22T18_57_33.048/working/TSKY0001.sb32504458.eb32521628.57608.19776135417_split.ms
output_dir
/lustre/aoc/cluster/pipeline/vlass_auto/spool/quicklook/Pilot_SGC3B_1.J235401+124236_P30566v1_2019_01_22T18_57_33.048/working
Start time
2019-01-24 09:50:47.227
End
2019-01-24 09:52:55.081
Duration
0:02:07.854
Note, WebLog generation is not included in the time.

CASA logs for stage 6